A Comprehensive Study of Infrared OH Prompt Emission in Two Comets. II. Implications for Unimolecular Dissociation of H2O

Astronomy and Astrophysics – Astronomy

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Comets: General, Comets: Individual (C/2000 Wm1 [Linear]), Comets: Individual (C/2004 Q2 [Machholz]), Molecular Data

Scientific paper

Infrared emission from hydroxyl has been observed in several comets via high-resolution infrared spectroscopy. The principal excitation mechanism for this emission is single-step photolysis of H2O, terminating in OH fragments that are both vibrationally and rotationally excited. Recently reported comet data provide quantitative measures of the rotational distribution of OH*[X2Π v'=1] for J'<17.5. The measured distributions of relative g-factors for OH ``prompt'' emission, and especially the ratios of the Π(A") and Π(A') Λ-doubling components, are remarkably similar for comets C/2000 WM1 (LINEAR) and C/2004 Q2 (Machholz). We discuss how these results complement ab initio theoretical studies of water dissociation and those done in terrestrial laboratories.

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